Thermal desorption of formamide and methylamine from graphite and amorphous water ice surfaces
Henda Chaabouni, Stephan Diana, Thanh Nguyen, and Fran\c{c}ois Dulieu

TL;DR
This study measures the desorption energies of formamide and methylamine from graphite and amorphous water ice surfaces, revealing their interactions and release behaviors relevant to astrophysical environments.
Contribution
It provides new quantitative data on the desorption energies and mechanisms of formamide and methylamine from interstellar ice analogues, enhancing understanding of their gas-phase presence.
Findings
Formamide desorbs around 176 K from both surfaces.
Methylamine desorbs below 100 K from graphite and after 120 K from water ice.
Over 95% of formamide diffuses through water ice to graphite.
Abstract
Formamide (NH2CHO) and methylamine (CH3NH2) are known to be the most abundant amine-containing molecules in many astrophysical environments. The presence of these molecules in the gas phase may result from thermal desorption of interstellar ices. The aim of this work is to determine the values of the desorption energies of formamide and methylamine from analogues of interstellar dust grain surfaces and to understand their interaction with water ice. TPD experiments of formamide and methylamine ices were performed in the submonolayer and monolayer regimes on graphite (HOPG) and non-porous amorphous solid water ice surfaces at 40-240 K. The desorption energy distributions of these two molecules were calculated from TPD measurements using a set of independent Polanyi-Wigner equations. The maximum of the desorption of formamide from both graphite and ASW ice surfaces occurs at 176 K after…
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